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银河系宇宙射线的 anisotropy 和 corotation 在银河系宇宙射线的 anisotropy 和 corotation 在银河系宇宙射线的
1Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan.
概括
研究人员使用西藏空气淋浴阵列测量了银河系宇宙射线的异质性. 在Cygnus地区附近发现了一种新的异性异性成分,在更高的能量下消失,表明宇宙射线与磁场的对应.
科学领域:
- 宇宙射线物理学 宇宙射线物理学
- 天体物理学 天体物理学
- 粒子天体物理学 粒子天体物理学
背景情况:
- 银河系宇宙射线由于银河系磁场的影响而表现出近同otropy.
- 了解宇宙射线异性质对于天体物理学和粒子物理学至关重要.
研究的目的:
- 为了呈现宇宙射线的高精度,二维异构性测量.
- 为了研究宇宙射线在几到几百特雷电子伏特 (TeV) 的能量上的行为.
- 为了发现宇宙射线异质性的新组成部分.
主要方法:
- 利用了来自西藏空气淋浴阵列的大数据集.
- 进行了宇宙射线的二维异构性测量.
- 分析了从几到几百TeV的能量数据.
主要成果:
- 揭示了先前已知的宇宙射线异质的细节.
- 发现了银河系宇宙射线在星际时间中的异构性的新组成部分,起源于天座区域.
- 在能量高达几百TeV时观察到所有异性质成分的色.
结论:
- 异构形的色表明银河系宇宙射线与当地的银河系磁环境在更高的能量下相结合.
- 这些发现影响了我们对宇宙射线,超新星,磁场和银河系动力学的理解.
- 这项研究为日球和银河系环境中的复杂相互作用提供了新的见解.
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